The optical reference information files have been updated to reflect the Phase A payload design. This is the design that is baselined for the upcoming System Requirements Review and Baseline Design Review.
» WFIRST Observatory Reference Information (.pptx) A compendium of basic information on the WFIRST Observatory, as of July 31, 2017.
» WFIRST Wide-Field Instrument Reference Information (.pptx) A compendium of basic reference information on the WFIRST Wide-Field Instrument, August 1, 2017
» WFIRST SRR: Data from WIM Model (.xlsm)
Point-spread functions for the WFIRST Wide-Field Instrument (aka 'Wide Field Camera') can be computed at any wavelength and at any position in the field of view, given knowledge of the pupil function. The file give Zernike decompositions of the wavefront error and pupil masks needed to perform this calculation.
» Explanation of Zernike coefficients (.docx) Contains the Zernike coefficients for the WFI, and also provides a fit to distortions in WFI imaging mode (WIM), a mapping of WIM detector positions onto the sky, WFI SCA positions in the focal plane, etc. Zernike coefficients are also provided for the grism Wide-Field Spectroscopy Mode (WSM) in first order, and for a single field position in 0th and 2nd order.
» Grism Mode SCA Projected Fields (.xlsx) This spreadsheet provides a calculator for each SCA giving the mapping in both directions between sky angle and wavelength to detector position.